Add to ORKGResults are presented from an extensive series of new high resolution scanning electron microscope studies of the very primative group of meteorites known as unequilibrated chondrites. These include quantitative analyses of micrometer sized phases and interpretation in terms of relevant phase equilibria. Several new meteorite minerals including high chromium metal, have been discovered
A wide range of analytical and experimental techniques were used to determine the nature and origin ...
Modifications to and maintenance of the JEOL 100 CX electron microscope are discussed. Research acti...
Several meteorites arrive on Earth every day, but only a small percentage of them are found. They ar...
Recent results on the antarctic meteorite ALPHA 77003 which contribute to understanding the alterati...
The evolution of the lunar regolith under solar wind and micrometeorite bombardment is discussed as ...
During a 13 year period beginning in 1971, the Extraterrestrial Petrology Group examined lunar soils...
Flameless atomic abosrption, X-ray photoemission spectroscopy, ferromagnetic resonance, scanning ele...
The data collection and the interpretation with respect to the mineralogy of meteoritic and terrestr...
Experimental and thermodynamic research on the pressure temperature limits of the stability of the m...
We present the results of the mineralogical and chemical analysis of a newly discovered lunar meteor...
MIL 090001 is a large (greater than 6 kg) CV chondrite from the reduced subgroup (CV(sub red)) that ...
Antarctic Meteorite ALHA 81005. This small, special meteorite has been the focus of much attention. ...
Metal particles from the Apollo 11 and 12 soil are both meteoritic and lunar in origin. In the Apoll...
Charged particle-induced nuclear reactions were used in the following problems: the determination o...
In the period named, P.I. Wood and his Research Associate M.I. Petaev published or submitted for pub...
A wide range of analytical and experimental techniques were used to determine the nature and origin ...
Modifications to and maintenance of the JEOL 100 CX electron microscope are discussed. Research acti...
Several meteorites arrive on Earth every day, but only a small percentage of them are found. They ar...
Recent results on the antarctic meteorite ALPHA 77003 which contribute to understanding the alterati...
The evolution of the lunar regolith under solar wind and micrometeorite bombardment is discussed as ...
During a 13 year period beginning in 1971, the Extraterrestrial Petrology Group examined lunar soils...
Flameless atomic abosrption, X-ray photoemission spectroscopy, ferromagnetic resonance, scanning ele...
The data collection and the interpretation with respect to the mineralogy of meteoritic and terrestr...
Experimental and thermodynamic research on the pressure temperature limits of the stability of the m...
We present the results of the mineralogical and chemical analysis of a newly discovered lunar meteor...
MIL 090001 is a large (greater than 6 kg) CV chondrite from the reduced subgroup (CV(sub red)) that ...
Antarctic Meteorite ALHA 81005. This small, special meteorite has been the focus of much attention. ...
Metal particles from the Apollo 11 and 12 soil are both meteoritic and lunar in origin. In the Apoll...
Charged particle-induced nuclear reactions were used in the following problems: the determination o...
In the period named, P.I. Wood and his Research Associate M.I. Petaev published or submitted for pub...
A wide range of analytical and experimental techniques were used to determine the nature and origin ...
Modifications to and maintenance of the JEOL 100 CX electron microscope are discussed. Research acti...
Several meteorites arrive on Earth every day, but only a small percentage of them are found. They ar...